The transformations that take place in late‐type galaxies in the environment of rich clusters
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …

We simulate the assembly of a massive rich cluster and the formation of its constituent
galaxies in a flat, low-density universe. Our most accurate model follows the collapse, the …

We use a complete sample of galaxies drawn from the Sloan Digital Sky Survey to study
how structure, star formation and nuclear activity depend on local density and on stellar …

We investigate the well-known correlations between the dynamical mass-to-light ratio (M/L)
and other global observables of elliptical (E) and lenticular (S0) galaxies. We construct two …

In Paper I of this series we introduced a volume-limited parent sample of 871 galaxies from
which we extracted the ATLAS3D sample of 260 early-type galaxies (ETGs). In Papers II and …

We take advantage of the largest high-resolution simulation of cosmic structure growth ever
carried out—the Millennium Simulation of the concordance Λ cold dark matter (CDM) …

We present in this paper a detailed analysis of the effect of environment on the star formation
activity of galaxies within the Early Data Release (EDR) of the Sloan Digital Sky Survey …

We have measured the equivalent width of the Hα emission line for 11 006 galaxies brighter
than M b=− 19 (ΩΛ= 0.7, Ω m= 0.3, H 0= 70 km s− 1 Mpc− 1) at 0.05< z< 0.1 in the 2dF …

We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled
independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey …

Using a large galaxy group catalogue constructed from the Sloan Digital Sky Survey Data
Release 2, we investigate the correlation between various galaxy properties and halo mass …